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<ri:Resource created="2017-11-27T14:13:32Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Photometry of LBGs, LAEs and GNBs at z~2.85</title><shortName>J/ApJ/779/65</shortName><identifier>ivo://CDS.VizieR/J/ApJ/779/65</identifier><altIdentifier>doi:10.26093/cds/vizier.17790065</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mostardi R.E.</name></creator><creator><name>Shapley A.E.</name></creator><creator><name>Nestor D.B.</name></creator><creator><name>Steidel C.C.</name></creator><creator><name>Reddy N.A.,Trainor R.F.</name></creator><date role="Updated">2018-04-04T05:52:56Z</date><date role="Created">2017-11-27T14:13:32Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>ultraviolet-photometry</subject><subject>redshifted</subject><description>We present results from a survey for z~2.85 Lyman-continuum (LyC) emission in the HS1549+1933 field and place constraints on the amount of ionizing radiation escaping from star-forming galaxies. Using a custom narrowband filter (NB3420) tuned to wavelengths just below the Lyman limit at z&gt;=2.82, we probe the LyC spectral region of 49 Lyman break galaxies (LBGs) and 91 Ly{alpha} emitters (LAEs) spectroscopically confirmed at z&gt;=2.82. Four LBGs and seven LAEs are detected in NB3420. Using V-band data probing the rest-frame nonionizing UV, we observe that many NB3420-detected galaxies exhibit spatial offsets between their LyC and nonionizing UV emission and are characterized by extremely blue NB3420-V colors, corresponding to low ratios of nonionizing to ionizing radiation (F_UV_/F_LyC_) that are in tension with current stellar population synthesis models. We measure average values of (F_UV_/F_LyC_) for our LBG and LAE samples, correcting for foreground galaxy contamination and H I absorption in the intergalactic medium. We find (F_UV_/F_LyC_)_corr_^LBG^=82+/-45 and (F_UV_/F_LyC_)_corr_^LAE^=7.4+/-3.6. These flux density ratios correspond, respectively, to relative LyC escape fractions of f_esc,rel_^LBG^=5%-8%, and f_esc,rel_^LAE^=18%-49% absolute LyC escape fractions of f_esc,rel_^LBG^=1%-2% and f_esc,rel_^LAE^=5%-15%, and a comoving LyC emissivity from star-forming galaxies of 8.8-15.0x10^24^ erg/s/Hz/Mpc^3^. In order to study the differential properties of galaxies with and without LyC detections, we analyze narrowband Ly{alpha} imaging and rest-frame near-infrared imaging, finding that while LAEs with LyC detections have lower Ly{alpha} equivalent widths on average, there is no substantial difference in the rest-frame near-infrared colors of LBGs or LAEs with and without LyC detections. These preliminary results are consistent with an orientation-dependent model where LyC emission escapes through cleared paths in a patchy interstellar medium.</description><source format="bibcode">2013ApJ...779...65M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/779/65</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/498/13">J/A+A/498/13 : Lyman-{alpha} emitters from redshifts z~2-3 (Nilsson+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/18">J/ApJ/736/18 : Lyman-continuum emission at z~3 in SSA22 field (Nestor+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/744/110">J/ApJ/744/110 : LAE galaxies between 2.1=&lt;z&lt;=3.1 (Ciardullo+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/47">J/ApJ/765/47 : Lyman-break galaxies and LAEs at z~3 (Nestor+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A142">J/A+A/563/A142 : UGR photometry of LBG candidates at z~3 (Boutsia+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/107">J/ApJ/810/107 : Lyman break galaxies and LAEs HST photometry (Mostardi+, 2015)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/779/65</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/779/65</mirrorURL><mirrorURL 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